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OACt OAC
OATs
METIS
Scientific Observing Modes
Science Activity Plan
Daniele Spadaro
INAF-Osservatorio Astrofisico di Catania
Italy
METIS Workshop
Göttingen, November 21st-23rd, 2018
OACt OAC
OATs
METIS
•Specific instrument observing modes have been defined
in order to address the scientific objective of METIS
investigation (see METIS-OACT-RPT-001)
•General METIS observations:
global maps of the coronal emission in UV H I Ly-α and
VL (580-640 nm range)
different spatial resolution and detector exposure time,
depending on the science goal and the instantaneous field
of view (FoV).
METIS
Timeline for the study of the high frequency
brightness fluctuations spectra (duration ~ 1 hr)
Minimum and maximum detectable frequencies
depending on duration and cadence of obs
METIS
• A revision of observing modes is in order:
also taking into account the discussions at the meeting,
the instrument calibration results and SW performance
• Observing modes will be the fundamental contribution
to the specific science activites constituting the
backbone of the Solar Orbiter Science Activity Plan
OACt OAC
OATs
METIS
https://issues.cosmos.esa.int/solarorbiterwiki/display/SOSP/SAP-related+work